关于单硫化离子体的光谱特性和线强度的理论研究
Guosen Wang1, Xinlu Cheng1, Hong Zhang2,3
1Institute of Atomic and Molecular Physics, Sichuan University, Chengdu 610065, China.
The journal of physical chemistry. A
|December 21, 2023
概括
这项研究计算了单硫化物 (SiS+),一种潜在的天体分子的光谱特性和光谱线强度. 结果为在星际空间中识别SiS+提供了关键数据.
科学领域:
- 天体化学是天体化学.
- 计算化学计算化学
- 频谱学是一种光谱学.
背景情况:
- 单硫化 (SiS+) 是一个潜在的天体分子.
- 对SiS+存在有限的光谱数据,这阻碍了其天文识别.
研究的目的:
- 计算SiS+的潜在能量曲线,二极极时刻和过渡二极时刻.
- 确定SiS+的光谱常数和光谱线强度.
主要方法:
- 使用了配置相互作用计算 (icMRCI + Q).
- 施罗丁格方程被解决以获得光谱常数.
- 分区函数和爱因斯坦系数被计算出来,以导出光谱线强度.
主要成果:
- 为SiS+的12个结合状态获得了光谱常数.
- 分区函数被计算为温度在300到10,000K之间.
- 对于X2Π和A2Σ+状态及其过渡的光谱线强度计算在300K和3000K.
结论:
- 这项研究为SiS+定位提供了重要的光谱数据.
- 这些数据将有助于在星际环境中检测和描述SiS+.
- 计算的光谱线强度显示了不同状态的温度依赖强度最大值.
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